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Spectroscopic Determination of the Phase Composition and Temperature of Nitrogen Ice on Triton
1 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125
Laboratory spectra of the first overtone band (2.1480 micrometers, 4655.4 reciprocal centimeters) of solid nitrogen show additional structure at 2.1618 micrometers (4625.8 reciprocal centimeters) over a limited temperature range. The spectrum of Neptune's satellite Triton shows the nitrogen overtone band as well as the temperature-sensitive component. The temperature dependence of this band may be used in conjunction with ground-based observations of Triton as an independent means of determining the temperature of surface deposits of nitrogen ice. The surface temperature of Triton is found to be 38.0+2.01.0 K, in agreement with previous temperature estimates and measurements. There is no spectral evidenceforthe presence of Accepted on June 3, 1993
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Science. ISSN 0036-8075 (print), 1095-9203 (online)